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The Relation of the Low Frequency Source to the Crab Pulsar

Published online by Cambridge University Press:  07 February 2017

Kenneth R. Lang
Kenneth R. Lang*
Affiliation:
Cornell-Sydney University Astronomy Center, Arecibo Observatory, Cornell University, Ithaca N.Y., U.S.A.

Abstract

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The view that the compact low frequency source and the pulsar NP 0532 are the same object is substantiated by an examination of the general properties of interstellar scattering. This scattering accounts for the observed angular size of the compact source, the observed pulse broadening of NP 0532, the continuum nature of the compact source, and the observed spectrum of both the pulsar and the compact source.

Type
Session 2
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 91 - 96
Copyright
Copyright © Reidel 1971 

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